Spatial density fluctuations in the radiation ERA of the universe

Details Spatial density fluctuations in the radiation ERA of the universe Spatial density fluctuations in the radiation ERA of the universe

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100..359l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 359-367.

Astronomy and Astrophysics

Astrophysics

1

Galactic Evolution, Relativistic Plasmas, Space Density, Universe, Big Bang Cosmology, Boltzmann Distribution, Cosmic Gases, Galactic Radiation, Temperature Distribution, Temperature Gradients

Scientific paper

It is shown that in the radiation era of the Universe spatial temperature fluctuations (ΔT/T) < 10-5 in the cosmic plasma lead to huge changes of density up to (Δρ/ρ) ≅ 104. This effect results from the fact that the cosmic plasma in the radiation era can be considered as a general relativistic Boltzmann gas which is found in the very vicinity of equilibrium.

Affiliated with

Also associated with

No associations

Rating

Spatial density fluctuations in the radiation ERA of the universe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spatial density fluctuations in the radiation ERA of the universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spatial density fluctuations in the radiation ERA of the universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1037005